17 Billion Earth-Size Alien Planets Inhabit Milky Way

This artist's illustration represents the variety of planets being detected by NASA's Kepler spacecraft. Scientists now say that one in six stars hosts an Earth-size planet.
(C. Pulliam & D. Aguilar (CfA))

This chart depicts the frequencies of planets based on findings from NASA's Kepler space observatory. The results show that one in six stars has an Earth-sized planet in a tight orbit.
(F. Fressin (CfA))

The Milky Way hosts at least 17 billion Earth-size alien planets, and probably many more, a new study reveals.

Astronomers have determined that about 17 percent of stars in our galaxy harbor a roughly Earth-size exoplanet in a close orbit. Since there are 100 billion or so stars in the Milky Way, that works out to a minimum of 17 billion small, rocky alien worlds, or an Earth-size planet around one of every six stars.

And there are probably many more such planets orbiting at greater distances from their stars, some of which may even be "alien Earths" capable of supporting life as we know it.

"These kind of rocky objects are everywhere," team member Francois Fressin, of the Harvard-Smithsonian Center for Astrophysics (CfA), told reporters today (Jan. 7) during a meeting of the American Astronomical Society in Long Beach, Calif. [The Strangest Alien Planets (Gallery)]

Kepler detects alien worlds by noting the telltale dips in brightness caused when planets cross the face of — or transit — their parent stars from the instrument's perspective. The telescope, which launched in March 2009, flagged more than 2,700 potential planets in its first 22 months of operation, more than 100 of which have been confirmed to date.

The research team wanted to know how complete and accurate Kepler's survey has been — that is, what percentage of its finds are real, and how many planets is it likely missing? So they came up with a simulation that mimicked the telescope's work, finding that about 90 percent of its detections are probably the real deal.

"There is a list of astrophysical configurations that can mimic planet signals, but altogether, they can only account for one-tenth of the huge number of Kepler candidates," Fressin said in a statement. "All the other signals are bona-fide planets."

The study has been accepted for publication in The Astrophysical Journal.

Planets, planets everywhere

Using information from both the actual and simulated Kepler surveys, the team calculated some estimates about how common different types of planets are thoughout the Milky Way.

They determined, for example, that 17 percent of stars have a planet 0.8 to 1.25 times the size of Earth in tight orbits, with periods of 85 days or less. About 25 percent of stars have a so-called "super-Earth" (worlds 1.25 to 2 times as big as our own) in an orbit of 150 days or less — the same percentage that hosts a "mini-Neptune" (a planet 2 to 4 times Earth's size) with an orbital period up to 250 days.

Big planets such as Saturn or Jupiter are far less common. Only 5 percent of stars harbor a gas giant with an orbital period of 400 days or less, researchers said.

Overall, the team found that about 50 percent of all stars in the Milky Way have a planet the size of Earth or larger in a tight orbit. Extrapolation and incorporation of data from other instruments suggest that virtually all sun-like stars host planets, Fressin said.

Further, stars don't have to be sun-like to host an Earth-size world. The team also determined that small and medium-size exoplanets are commonly found around red dwarfs as well, which are smaller and cooler than our star.

"Earths and super-Earths aren’t picky," said co-author Guillermo Torres, also of the CfA. "We’re finding them in all kinds of neighborhoods."

Kepler generally requires three planetary transits to flag a potential alien world. Since more tightly orbiting planets transit more frequently, the telescope's early findings have been biased toward close-in worlds. But as Kepler continues to operate, it should find more and more planets farther from their host stars — including, perhaps, Earth-size worlds in Earthlike orbits.